Fig. 4

Comparison of disk inclinations derived with Galfit (iGALFIT) for the MUSE-HDFS spatially resolved galaxies and previous measurements (iT04) performed by Trujillo & Aguerri (2004). Green dotted lines are for iGALFIT = 0 and iT04 = 0. Dots are color-coded as a function of the relative size of the disk (effective radius derived from Galfit) with respect to the MUSE PSF FWHM. Labels indicate the galaxy ID.
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